Ammonia abundance in Jupiter's atmosphere derived from the attenuation of the Galileo probe's radio signal

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Abstract

The radio signal from the Galileo probe to the orbiter experienced attenuation due to ammonia in Jupiter's atmosphere during the probe descent. A profile of the ammonia content as a function of depth in the atmosphere has been derived from the measurements of the attenuation. The derived ammonia abundance rises to a molar fraction of 700 ±100 parts per million for pressures greater than 7 bars, about 4 times that expected based on the solar abundance of nitrogen. Copyright 1998 by the American Geophysical Union.

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Folkner, W. M., Woo, R., & Nandi, S. (1998). Ammonia abundance in Jupiter’s atmosphere derived from the attenuation of the Galileo probe’s radio signal. Journal of Geophysical Research: Planets, 103(E10), 22847–22855. https://doi.org/10.1029/98JE01635

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